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Volume 35 Issue 2
Apr 2024
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Lin Liang, Guibin Zhang, Shengxuan Huang, Jingjing Niu, Dongzhou Zhang, Jingui Xu, Wen Liang, Shan Qin. High-Pressure Behavior of Ferromagnesite (Mg0.81Fe0.19)CO3 by Synchrotron X-Ray Diffraction and Raman Spectroscopy up to 53 GPa. Journal of Earth Science, 2024, 35(2): 525-535. doi: 10.1007/s12583-021-1495-y
Citation: Lin Liang, Guibin Zhang, Shengxuan Huang, Jingjing Niu, Dongzhou Zhang, Jingui Xu, Wen Liang, Shan Qin. High-Pressure Behavior of Ferromagnesite (Mg0.81Fe0.19)CO3 by Synchrotron X-Ray Diffraction and Raman Spectroscopy up to 53 GPa. Journal of Earth Science, 2024, 35(2): 525-535. doi: 10.1007/s12583-021-1495-y

High-Pressure Behavior of Ferromagnesite (Mg0.81Fe0.19)CO3 by Synchrotron X-Ray Diffraction and Raman Spectroscopy up to 53 GPa

doi: 10.1007/s12583-021-1495-y
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  • Corresponding author: Shan Qin, sqin@pku.edu.cn
  • Received Date: 23 Apr 2021
  • Accepted Date: 09 Jun 2021
  • Available Online: 11 Apr 2024
  • Issue Publish Date: 30 Apr 2024
  • Ferromagnesite (Mg, Fe)CO3 with 20 mol% iron is a potential host mineral for carbon transport and storage in the Earth mantle. The high-pressure behavior of synthetic ferromagnesite (Mg0.81Fe0.19)CO3 up to 53 GPa was investigated by synchrotron X-ray diffraction (XRD) and Raman spectroscopy. The iron bearing carbonate underwent spin transition at around 44–46 GPa accompanied by a volume collapse of 1.8%, which also demonstrated a variation in the dνi/dP slope of the Raman modes. The pressure-volume data was fitted by a third-order Birch-Murnaghan equation of state (BM-EoS) for the high spin phase. The best-fit K0 = 108(1) GPa and $ {\mathit{K}}_{0}^{\mathbf{'}} $ = 4.2(1). Combining the dνi/dP and the K0, the mode Grüneisen parameters of each vibrational mode (T, L, ν4 and ν1) were calculated. The effects of iron concentration on the Mg1-xFexCO3 system related to high-pressure compressibility and vibrational properties are discussed. These results expand the knowledge of the physical properties of carbonates and provide insights to the potential deep carbon host.

     

  • Electronic Supplementary Materials: Supplementary materials (Figures S1–S6; Supplementary Material A) are available in the online version of this article at https://doi.org/10.1007/s12583-021-1495-y.
    Conflict of Interest
    The authors declare that they have no conflict of interest.
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